Solar variability in the CaII K during solar cycles 21 and 22

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1578

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.contributor.author	Gupta, S. S	-
dc.contributor.author	Kariyappa, R	-
dc.contributor.author	Aleem, P. S. M	-
dc.contributor.author	Sundararaman, K	-
dc.date.accessioned	2007-05-10T09:08:48Z	-
dc.date.available	2007-05-10T09:08:48Z	-
dc.date.issued	1993	-
dc.identifier.citation	BASI, Vol. 21, pp. 655-657	en
dc.identifier.uri	http://hdl.handle.net/2248/1578	-
dc.description.abstract	We have monitored the sun in the light of the CaII K line and obtained the disc integrated profiles for the years 1974-91. From these profiles we have estimated the variability of the sun as a star as seen in the various K line parameters. The 1 A index shows an increase of about 35% in 1990 from its minimum value attained in 1986-87.	en
dc.format.extent	164468 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Solar variability	en
dc.title	Solar variability in the CaII K during solar cycles 21 and 22	en
dc.type	Article	en
Appears in Collections:	BASI Publications IIAP Publications

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